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Reference: Rostek C, et al. (2008) Involvement of homologous recombination repair after proton-induced DNA damage. Mutagenesis 23(2):119-29

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Abstract

Protection from chronic exposure to cosmic radiation, which is primarily composed of protons, in future manned missions to Mars and beyond is considered to be a key unresolved issue. To model the effects of cosmic radiation on a living cell, we used Saccharomyces cerevisiae cells harboring various deletions of DNA repair genes to investigate the response of cells to DNA strand breaks caused by exposure to 250 MeV proton irradiation (linear energy transfer of 0.41 keV/mum). In our study, DNA strand breaks induced by exposure to protons were predominantly repaired via the homologous recombination and postreplication repair pathways. We simulated chronic exposure to proton irradiation by treating cells from colonies that survived proton treatment, after several rounds of subculturing, to a second proton dose, as well as additional cell stressors. In general, cells cultured from proton surviving colonies were not more sensitive to secondary cell stressors. However, cells from rad52Delta colonies that survived proton treatment showed increased resistance to secondary stressors, such as gamma-rays (1.17 and 1.33 MeV; 0.267 keV/mum), ultraviolet (UV) and proton irradiation and elevated temperatures. Resistance to secondary stressors was also observed in rad52Delta cells that survived exposure to gamma-rays, rather than protons, but this was not observed to occur in rad52Delta cells after UV irradiation. rad52Delta cells that survived exposure to protons, followed by gamma-rays (proton surviving colonies were cultured prior to gamma-ray exposure), exhibited an additive effect, whereby these cells had a further increase in stress resistance. A genetic analysis indicated that increased stress resistance is most likely due to a second-site mutation that suppresses the rad52Delta phenotype. We will discuss possible origins of these second-site mutations.

Reference Type
Journal Article
Authors
Rostek C, Turner EL, Robbins M, Rightnar S, Xiao W, Obenaus A, Harkness TA
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